The Snow Line in Viscous Disks Around Low-Mass Stars: Implications for Water Delivery to Terrestrial Planets in the Habitable Zone

Astrophysical Journal - United States
doi 10.1088/0004-637x/807/1/9
Full Text
Abstract

Available in full text

Date
Authors
Publisher

IOP Publishing

Related search

Terrestrial Planets and Water Delivery Around Low-Mass Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

Water Delivery by Pebble Accretion to Rocky Planets in Habitable Zones in Evolving Disks

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Water in the Envelopes and Disks Around Young High-Mass Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

The Basic Principles of Creation of Habitable Planets Around Stars in the Milky Way Galaxy

International Journal of Astronomy and Astrophysics
2016English

The Detection of Earth-Mass Planets Around Active Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Detectability of Atmospheric Features of Earth-Like Planets in the Habitable Zone Around M Dwarfs

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Tidal Dissipation in Rotating Low-Mass Stars and Implications for the Orbital Evolution of Close-In Massive Planets

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Demographics of Disks Around Young Very Low-Mass Stars and Brown Dwarfs in Lupus

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2020English

The Stability of the Orbits of Earth-Mass Planets in the Habitable Zone of 47 Ursae Majoris

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2002English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy